The solar burst of 13 July, 1986 at 2I cm wavelength was recorded with a time constant of 8 ms. In the course of the burst lasting for about 40 min there appeared distinct stages of the burst's evolution. They consisted of the pattern of energy release in flares which was proposed by Sturrock et al.
โฆ LIBER โฆ
Dual pulsations in solar radio bursts at short centimeter wavelengths
โ Scribed by Zhihai Qin; Chunseng Li; Qijun Fu; Zhengmin Gao
- Publisher
- Springer
- Year
- 1996
- Tongue
- English
- Weight
- 693 KB
- Volume
- 163
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
โฆ Synopsis
It is well known that the oscillating MHD waves drive periodic variations in the magnetic field. But how the MHD waves can be triggered in the flaring loops is not yet well known. It seems to us that this problem should be connected with the physical processes occurring in the flare loop during a solar flare. A peculiar solar flare event at 04:00-04:51 UT on May 23, 1990 was observed simultaneously with time resolutions 1 s and
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